Search Publications

Revisiting the Suzaku spectrum of the Galactic SNR W 49B: Non-detection of iron K-shell charge-exchange emission and refined ejecta-mass ratios of iron-group elements
DOI: 10.1093/pasj/psaf012 Bibcode: 2025PASJ...77..446S

Sato, Toshiki; Sawada, Makoto; Maeda, Keiichi +1 more

The origin of the recombining plasma in several Galactic SNRs has been debated. A plausible mechanism would be a rapid cooling in the past, by either an adiabatic or a conductive process. A recent spectral study of W 49B reported a possible charge-exchange emission due to collisions between the shock-heated ejecta and cold clouds, which could be d…

2025 Publications of the Astronomical Society of Japan
Suzaku 1
Suzaku Observations of the Cold Front in A3667: A Nonequilibrium Ionization State of the Intracluster Medium
DOI: 10.3847/1538-4357/ad96ac Bibcode: 2025ApJ...979...47S

Kohmura, Takayoshi; Uchida, Yuusuke; Shishido, Mona

We present a systematic study of the thermodynamic properties of the intracluster medium (ICM), including the plasma conditions in the ICM, in the merging galaxy cluster A3667 using Suzaku. We analyze the X-ray spectra of the ICM between the northwestern and the southeastern radio relics across a prominent cold front in A3667 to search for the ICM…

2025 The Astrophysical Journal
Suzaku XMM-Newton 0
An X-ray study of changing-look active galactic nuclei
DOI: 10.1051/0004-6361/202451098 Bibcode: 2025A&A...693A.126T

Titarchuk, Lev; Seifina, Elena; Mishin, Egor

A significant number of changing-look active galactic nuclei (CL AGNs) have been identified to date. In this work, we study what happens to the X-ray spectrum during CL events. We use the example of the nearby CL Seyfert named NGC 1566, which has been observed by Swift, NuSTAR, XMM-Newton, and Suzaku. We applied the Comptonization model to describ…

2025 Astronomy and Astrophysics
Suzaku XMM-Newton 0
Pulse-profile Modeling and Spin–Orbit Alignment in a Suzaku Sample of Accreting X-Ray Binary Pulsars
DOI: 10.3847/1538-4357/ad9399 Bibcode: 2025ApJ...978...80L

Paul, Biswajit; Laycock, Silas G. T.; Pradhan, Pragati +2 more

We report pulse-profile modeling of a sample of 23 X-ray binary pulsars observed with the Suzaku X-ray satellite. These pulsars have spin periods ranging from 0.7 to 9400 s, and their X-ray emission is powered by the accretion from their stellar companions. We fitted each individual pulse profile with the Polestar geometric model, which accounts f…

2025 The Astrophysical Journal
Suzaku 0